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Dark Matter

OCR A-level PhysicsAstrophysics and CosmologyLesson 23 of 24

Dark matter is matter that does not emit or absorb electromagnetic radiation, so it cannot be seen directly. We know it is there only because of its gravitational effects on visible matter.

The main evidence comes from the rotation curves of spiral galaxies. A rotation curve is a graph of the orbital speed of stars against their distance from the centre of the galaxy.

Diagram

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